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Implications of Directed Energy for SETI

机译:定向能对SETI的影响

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We compute the detectability of directed energy sources from distant civilizations that may exist. Recent advances in our own directed energy abilities allow us to foresee our own capability that will radically change our ability to broadcast our presence and hence allow us to ponder the reverse case of detection. In the next few decades we will evolve to the point where we will be able to produce the brightest SED (spectral energy distribution) in the known universe. We show that systems of this type have the ability to be detected at vast distances and indeed can be detected across the entire horizon. This profoundly changes the possibilities for searches for extra-terrestrial technology advanced civilizations. Even modest searches are extremely effective at detecting or limiting many civilization classes. For example, even a single civilization anywhere in our galaxy that is of comparable technological advancement to our own can be detected with near unity probability with a small cluster of 0.1 m telescopes on Earth while a 1 m class telescope has the ability to detect even a single civilization anywhere in the Andromeda galaxy. We compare ground based surveys with aperture sizes from 1mm (smaller than a cell phone optic) to 1 m (modest telescope) and compute blind transmission and blind reception probabilities. We propose a search strategy, using small Earth based telescopes, that will observe more than 10~(12) stellar and planetary systems with possible extensions to more than 10~(20) systems allowing us to test the hypothesis that other similarly or more advanced civilization with this same capability, and are broadcasting, exist. We show that such searches have unity probability of detecting even a single comparably advanced civilization anywhere in our galaxy within a relatively short search time (few years) IF that civilization adopts a simple beacon strategy we call "intelligent targeting", IF that civilization is beaconing at a wavelength we can detect and IF that civilization left the beacon on long enough for the light to reach us now. In this blind beacon and blind search strategy the civilization does not need to know where we are nor do we need to know where they are. This same basic strategy can be extended to extragalactic distances. Portions of this paper come from our recent paper entitled "The Search for Directed Intelligence".
机译:我们计算可能存在的遥远文明对定向能源的可探测性。我们自身定向能量能力的最新进展使我们能够预见自己的能力,这将从根本上改变我们广播存在状态的能力,从而使我们能够思考相反的探测情况。在接下来的几十年中,我们将发展到能够在已知宇宙中产生最亮的SED(光谱能量分布)的地步。我们表明,这种类型的系统具有在远距离检测的能力,并且实际上可以在整个范围内检测到。这深刻地改变了寻找地外技术先进文明的可能性。即使是适度的搜索,对于发现或限制许多文明类别也极为有效。例如,即使是在我们银河系中任何一个具有与我们自己相当的技术进步水平的文明,也可以用地球上0.1 m望远镜的小集群以接近统一的概率检测到,而1 m类望远镜甚至可以检测到仙女座星系中任何地方的单一文明。我们比较孔径从1mm​​(小于手机光学元件)到1m(普通望远镜)的地面测量,并计算盲发射和盲接收概率。我们提出了一种使用小型地球望远镜的搜索策略,该策略将观测超过10〜(12)个恒星和行星系统,并可能扩展到超过10〜(20)个系统,从而使我们能够检验其他类似或更高级的假设具有相同能力并正在传播的文明。我们表明,如果文明采用了一种简单的信标策略(我们称之为“智能目标定位”)(如果文明正在信标的话),那么这种搜索具有在相对较短的搜索时间(数年)内检测到星系中任何一个相对先进的文明的统一概率。在一个波长下,我们可以检测到,如果文明已经将信标留在足够长的时间,以至于现在光到达我们的身旁。在这种盲目信标和盲目搜索策略中,文明既不需要知道我们在哪里,也不需要知道它们在哪里。相同的基本策略可以扩展到银河外距离。本文的部分内容来自我们最近发表的题为“针对有向情报的搜索”的文章。

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